82 



Herman Schultz, 



li590 am the brightest of 4 th order; N v indistinct seems to consist of sev S *..,but 

 not to be decided, as the sky v dull; * 10 m f, and sev more *... nr. 



1. 50, L57 form the two nuclei of a continuous oval neby with 2 separate condens. 

 Tbe diagr in Ph Tr 33 consequently gives no exact idea of this object ; the diagr 

 by R seems on the contrary to be a faithful image of the neb. Both N are nr 

 on the axis of the neb: 1.56 nr central, pretty B; 1.57 nr the n edge, through 

 its faintness scarcely observable. N 1.56, E nr in the decl-circle, evidently r in 

 2 or 3 stellar points. State of the air only tolerable, and not more than 210 

 times magn. p. applicable. 



I1OO8 ; Nova; h009. 



hOOS F but conspicuous traces of r; ab E in the par; * 10 ,n sf. Sky v serene. 

 Nova eF; f hOOS some seconds ab 2' n; but not observable. 



hOOO hardly Fr than h608! Neb ab '/./; E nr in the decl-circle; * I0 m ,3 np. The 

 circumstance, that obs is scarcely troubled by the B * nr, prooves best, that 

 even this neb is pretty B. 



Rem. Are the objects in this region var? The two neb are evidently Br 

 than for instance 11.110 and h682, and consequently much Br than is to be 

 exspected according to the catalogues. The * BB. 10°2019, f h608 ab 40 s nr in 

 the par, is on the contrary only 10 m , and consequently Fr than according to BB. 



liG22 C condens uncertain: once seen with well defined N, once rM. 



1024: not much Fr than It 022. Is there a vvF neb immediately s? 



Ii027 is nowise eF, but obs diffic through the vicinity of *a 10 m p nr in the par. 



Astonishing, that this neb was not seen by D'A, and that h has not remarked 



the B *? 



GC. 1910 -R. Nova vvF, v diffic for obs especially as the sky much illuminated from 



B uorthernlight. 

 Ii034 Fr and Sr than h636 ; * I2 m sf. 

 It 030 in a trap of 4 *... 11™, 



h045 well seen; not particularly B and certainly not CI. I; diam in the decl-circle nr 

 '/./; rr with magn. p. 210, sev distinct *... 12"'13 especially in the nf part; *a 

 10 m ll sf. 



Rein. Other observers have not seen the neb resolved, and probably in 

 consequence thereof have found the neb Br than I have? D'A for instance has: 

 "Multum lucis, prima? manifesto classis etiamnunc ... . Ad amplificationem 226 

 nebula non dissolvitur." 



IV. 79= M. 82 E in pos 294° to 5' a 6', ab 1' br; neb has a condens of ab '/ 4 ' diam 

 in the nf part, and the place refers to the C of it; *... glimmering in and around 

 that condens spot. 



